AbstractWe apply the generalized second law of thermodynamics to discriminate among quantum corrections (whether logarithmic or power-law) to the entropy of the apparent horizon in spatially Friedmann–Robertson–Walker universes. We use the corresponding modified Friedmann equations along with either Clausius relation or the principle of equipartition of the energy to set limits on the value of a characteristic parameter entering the said corrections
We have considered that the universe is the inhomogeneous (n+2)-dimensional quasi-spherical Szekeres...
Abstract. In this paper we have considered the holographic dark energy and studied it’s cosmology an...
A new method is given for proving the semiclassical generalized second law (GSL) of horizon thermody...
Using the corrected entropy-area relation motivated by the loop quantum gravity, we investigate the ...
In the previous analyses in the literature about the generalized second law (GSL) in an accelerated ...
We discuss the generalized second law (GSL) and the constraints imposed by it for two types of Fried...
We investigate the generalized second law (GSL) and the constraints imposed by it for two types of F...
In this work, we have considered the power-law correction of entropy on the horizon. If the flat FRW...
We investigate the validity of the generalized second law of thermodynamics, applying Barrow entropy...
Abstract We investigate the validity of the generalized second law of thermodynamics, applying Barro...
Jacob Bekenstein's identification of black hole event horizon area with entropy proved to be a landm...
Jacob Bekenstein’s identification of black hole event horizon area with entropy proved to be a landm...
The generalized second law of thermodynamics states that entropy always increases when all event hor...
In this work, we have considered a non-canonical scalar field dark energy model in the framework of ...
The generalized second law of thermodynamics states that entropy always increases when all event hor...
We have considered that the universe is the inhomogeneous (n+2)-dimensional quasi-spherical Szekeres...
Abstract. In this paper we have considered the holographic dark energy and studied it’s cosmology an...
A new method is given for proving the semiclassical generalized second law (GSL) of horizon thermody...
Using the corrected entropy-area relation motivated by the loop quantum gravity, we investigate the ...
In the previous analyses in the literature about the generalized second law (GSL) in an accelerated ...
We discuss the generalized second law (GSL) and the constraints imposed by it for two types of Fried...
We investigate the generalized second law (GSL) and the constraints imposed by it for two types of F...
In this work, we have considered the power-law correction of entropy on the horizon. If the flat FRW...
We investigate the validity of the generalized second law of thermodynamics, applying Barrow entropy...
Abstract We investigate the validity of the generalized second law of thermodynamics, applying Barro...
Jacob Bekenstein's identification of black hole event horizon area with entropy proved to be a landm...
Jacob Bekenstein’s identification of black hole event horizon area with entropy proved to be a landm...
The generalized second law of thermodynamics states that entropy always increases when all event hor...
In this work, we have considered a non-canonical scalar field dark energy model in the framework of ...
The generalized second law of thermodynamics states that entropy always increases when all event hor...
We have considered that the universe is the inhomogeneous (n+2)-dimensional quasi-spherical Szekeres...
Abstract. In this paper we have considered the holographic dark energy and studied it’s cosmology an...
A new method is given for proving the semiclassical generalized second law (GSL) of horizon thermody...